The primary energy of the ultra‐high energy cosmic rays(UHECR) are measured with the number of fluorescence photons which are detected with fluorescence detectors(FD) in the Telescope Array experiment(TA). Howevery since there is large uncertinty as 19% in the measurement of the energy scale, the most important theme is improvement of the energy calibration. The electron light source(ELS) is a small electron linear accelerator for new energy calibration. The ELS is located 100 m far from the FD station, and injects electron beam which is accelerated to 40 MeV energy into the sky. We can calibrate the FD energy scale by detection the air shower directly which is generated by the electron beam. The ELS was developed in KEK Japan, and moved to the TA site in March 2009. We started the beam operation in September 2010, in consequence we detected the air shower which was generated by electron beam in the air. The output kinetic energy of the electron beam was 41.1 MeV, we adjusted the output charge from 40 to 140 pC/pulse. We expect that we can improve the uncertinty of the energy scale to about 10% with the ELS, futhermore ELS will be a very useful apparatus for R&D of future UHECR observation.
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22 September 2011
INTERNATIONAL SYMPOSIUM ON THE RECENT PROGRESS OF ULTRA‐HIGH ENERGY COSMIC RAY OBSERVATION
10–12 December 2010
Aichi, (Japan)
Research Article|
September 22 2011
Absolute energy calibration of FD by an electron linear accelerator for Telescope Array Available to Purchase
T. Shibata;
T. Shibata
aICRR, University of Tokyo, 5‐1‐5 Kashiwanoha, Kashiwa, Chiba(277‐8582), Japan
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A. Enomoto;
A. Enomoto
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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S. Fukuda;
S. Fukuda
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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M. Fukushima;
M. Fukushima
aICRR, University of Tokyo, 5‐1‐5 Kashiwanoha, Kashiwa, Chiba(277‐8582), Japan
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K. Furukawa;
K. Furukawa
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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D. Ikeda;
D. Ikeda
aICRR, University of Tokyo, 5‐1‐5 Kashiwanoha, Kashiwa, Chiba(277‐8582), Japan
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M. Ikeda;
M. Ikeda
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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H. Iwase;
H. Iwase
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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K. Kakihara;
K. Kakihara
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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T. Kamitani;
T. Kamitani
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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Y. Kondo;
Y. Kondo
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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J. N. Matthews;
J. N. Matthews
cUniversity of Utah, 115S, 1400E, Salt Lake City, UT(4112‐0830), US
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S. Ogio;
S. Ogio
dOsaka City University, 3‐3‐138 Sugimotocho, Sumiyoshiku, Osaka(558‐8585), Japan
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S. Ohsawa;
S. Ohsawa
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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H. Sagawa;
H. Sagawa
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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T. Sanami;
T. Sanami
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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M. Satoh;
M. Satoh
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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T. Shidara;
T. Shidara
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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T. Sugimura;
T. Sugimura
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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M. Yoshida;
M. Yoshida
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
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The Telescope Array Collaboration
The Telescope Array Collaboration
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T. Shibata
a
A. Enomoto
b
S. Fukuda
b
M. Fukushima
a
K. Furukawa
b
D. Ikeda
a
M. Ikeda
b
H. Iwase
b
K. Kakihara
b
T. Kamitani
b
Y. Kondo
b
J. N. Matthews
c
S. Ogio
d
S. Ohsawa
b
H. Sagawa
b
T. Sanami
b
M. Satoh
b
T. Shidara
b
T. Sugimura
b
M. Yoshida
b
The Telescope Array Collaboration
aICRR, University of Tokyo, 5‐1‐5 Kashiwanoha, Kashiwa, Chiba(277‐8582), Japan
bHigh Energy Accelerator Research Organization, 1‐1 Oho, Tsukuba, Ibaraki(305‐0801), Japan
cUniversity of Utah, 115S, 1400E, Salt Lake City, UT(4112‐0830), US
dOsaka City University, 3‐3‐138 Sugimotocho, Sumiyoshiku, Osaka(558‐8585), Japan
AIP Conf. Proc. 1367, 44–49 (2011)
Citation
T. Shibata, A. Enomoto, S. Fukuda, M. Fukushima, K. Furukawa, D. Ikeda, M. Ikeda, H. Iwase, K. Kakihara, T. Kamitani, Y. Kondo, J. N. Matthews, S. Ogio, S. Ohsawa, H. Sagawa, T. Sanami, M. Satoh, T. Shidara, T. Sugimura, M. Yoshida, The Telescope Array Collaboration; Absolute energy calibration of FD by an electron linear accelerator for Telescope Array. AIP Conf. Proc. 22 September 2011; 1367 (1): 44–49. https://doi.org/10.1063/1.3628713
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